Garchinger Maier-Leibnitz-Kolloquium: A decade of cosmological tensions from galaxy surveys
by
Lecture Hall, ground floor (west)
LMU building, Am Coulombwall 1, campus Garching
In the past decade, telescope observations of large areas of the sky containing large numbers of distant galaxies have been developed into the most powerful way to answer some of the most pressing questions in fundamental physics: the nature of dark energy (the accelerating force of cosmic expansion), dark matter (the main source of gravitational attraction in the cosmos), and neutrinos (arguably the oddest among the particles in the standard model). As we enter the next decade of galaxy surveys, the Dark Energy Spectroscopic Experiment (DESI) is using 5000 robotic fiber-based spectrographs on the Mayall Telescope at Kitt Peak, Arizona, to lead the field of precision measurements of the expansion history of the cosmos. As I will discuss in my talk, early results from DESI may have revealed, may have widened, or may have contributed to healing, a number of cracks in the standard model of cosmological physics, with interesting degeneracies between neutrino mass and dark energy equation of state and great prospects for discovery in the decade ahead of us.
Hybrid access via ZOOM:
https://lmu-munich.zoom.us/j/98457332925?pwd=TWc3V1JkSHpyOTBPQVlMelhuNnZ1dz09
Meeting ID: 984 5733 2925
Passcode: 979953
Peter Thirolf (LMU) / Norbert Kaiser (TUM)